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dc.contributor.authorPetrova, E. V.en
dc.contributor.authorGrokhovsky, V. I.en
dc.date.accessioned2020-10-20T16:36:47Z-
dc.date.available2020-10-20T16:36:47Z-
dc.date.issued2019-
dc.identifier.citationPetrova E. V. High pressure impacts on meteorites / E. V. Petrova, V. I. Grokhovsky. — DOI 10.1515/pac-2018-1119 // Pure and Applied Chemistry. — 2019. — Vol. 11. — Iss. 91. — P. 1857-1867.en
dc.identifier.issn0033-4545-
dc.identifier.otherhttps://doi.org/10.1515/pac-2018-1119pdf
dc.identifier.other1good_DOI
dc.identifier.othere98a28a1-070e-445e-a49e-c0fbdaf54e66pure_uuid
dc.identifier.otherhttp://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=85075488929m
dc.identifier.urihttp://elar.urfu.ru/handle/10995/92679-
dc.description.abstractIn the invited article, we review observations on changes in meteorite texture relevant to the early stages of formation of the Solar System based on the experimental shock wave loading of the material at the laboratory. Investigation of the physical and structural properties of high-pressure impacts on meteorites is important for few reasons, such as: Protection of the Earth from the near-Earth objects (NEOs); Study of processes that cannot yet be achieved under laboratory conditions; Understanding of conditions for asteroid mining. © 2019 IUPAC & De Gruyter. This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License. For more information, please visit: http://creativecommons.org/licenses/by-nc-nd/4.0/2019.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherDe Gruyteren
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourcePure and Applied Chemistryen
dc.subjectFORMATIONen
dc.subjectHTMC-XVIen
dc.subjectMETEORITESen
dc.subjectSHOCK EXPERIMENTen
dc.subjectSHOCK FEATURESen
dc.subjectSTRUCTUREen
dc.subjectMETEORITESen
dc.subjectSHOCK WAVESen
dc.subjectSTRUCTURE (COMPOSITION)en
dc.subjectTEXTURESen
dc.subjectFORMATIONen
dc.subjectHIGH PRESSUREen
dc.subjectHTMC-XVIen
dc.subjectLABORATORY CONDITIONSen
dc.subjectNEAR EARTH OBJECTSen
dc.subjectSHOCK FEATURESen
dc.subjectSHOCK-WAVE LOADINGen
dc.subjectMETEOR IMPACTSen
dc.titleHigh pressure impacts on meteoritesen
dc.typeConference Paperen
dc.typeinfo:eu-repo/semantics/conferenceObjecten
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1515/pac-2018-1119-
dc.identifier.scopus85075488929-
local.affiliationUral Federal University, Institute of Physics and Technology, Ekaterinburg, Russian Federation
local.contributor.employeePetrova, E.V., Ural Federal University, Institute of Physics and Technology, Ekaterinburg, Russian Federation
local.contributor.employeeGrokhovsky, V.I., Ural Federal University, Institute of Physics and Technology, Ekaterinburg, Russian Federation
local.description.firstpage1857-
local.description.lastpage1867-
local.issue91-
local.volume11-
local.identifier.pure11331730-
local.identifier.eid2-s2.0-85075488929-
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